Values of Nside for foreground parameter variations in three different 20% large regions of the sky. The Nside values are chosen to capture most of the spatial variability of the spectral indices and to keep the resulting foreground bias under control while not increasing the statistical uncertainty. The angular resolution for βd is kept to the maximum allowed (Nside = 64), since LiteBIRD turns out to be particularly sensitive to this parameter.
. | Galactic latitude . | ||
---|---|---|---|
. | Low . | Medium . | High . |
βd | 64 | 64 | 64 |
Td | 8 | 4 | 0 |
βs | 4 | 2 | 2 |
. | Galactic latitude . | ||
---|---|---|---|
. | Low . | Medium . | High . |
βd | 64 | 64 | 64 |
Td | 8 | 4 | 0 |
βs | 4 | 2 | 2 |
Values of Nside for foreground parameter variations in three different 20% large regions of the sky. The Nside values are chosen to capture most of the spatial variability of the spectral indices and to keep the resulting foreground bias under control while not increasing the statistical uncertainty. The angular resolution for βd is kept to the maximum allowed (Nside = 64), since LiteBIRD turns out to be particularly sensitive to this parameter.
. | Galactic latitude . | ||
---|---|---|---|
. | Low . | Medium . | High . |
βd | 64 | 64 | 64 |
Td | 8 | 4 | 0 |
βs | 4 | 2 | 2 |
. | Galactic latitude . | ||
---|---|---|---|
. | Low . | Medium . | High . |
βd | 64 | 64 | 64 |
Td | 8 | 4 | 0 |
βs | 4 | 2 | 2 |
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